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Fantom [35]
4 years ago
6

What does the zeroth law of thermodynamics allow us to define?

Physics
2 answers:
LekaFEV [45]4 years ago
6 0
<h2>Answer:</h2>

<u>The correct choice is </u><u>D.  thermal energy</u>

<h2>Explanation:</h2>

According to the zeroth law of thermodynamics, if two thermodynamic systems are each in thermal equilibrium with a third one, then they are in thermal equilibrium with each other. Accordingly, thermal equilibrium between systems is a transitive relation.Hence option D is the right answer

Rasek [7]4 years ago
5 0

Answer: D

Explanation:

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Newton's second law:

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Compare blue and red light from the visible spectrum. which has: the longer wavelength? the greater frequency? the greater energ
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1) By looking at the table of the visible spectrum, we see that blue light has a wavelength in the range [450-490 nm], while red light has wavelength in the range [620-750 nm]. Therefore, red light has longer wavelength than blue light.

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f= \frac{c}{\lambda}
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E=hf
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How far did a car travel if it was on the road for 55.2s and it traveled at an average speed of 55m/s
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A newly discovered planet is found to have a density if 2/3pe and a radius of 2RE, where PE and RED are the density and radius o
Liono4ka [1.6K]
Missing question in the text of the exercise. Found on internet:
"What is the acceleration due to gravity on the surface of the planet?"

Solution:
The gravitational acceleration at Earth's surface is given by:
g= \frac{GM}{r^2} 
where
G is the gravitational constant
M is the Earth's mass
r is the Earth's radius

The Earth's mass can be rewritten also as the product between the Earth's density, d, and its volume (the volume of a sphere of radius r):
M=dV=d ( \frac{4}{3} \pi r^3)=  \frac{4}{3} \pi d r^3 

Now let's call M' the mass of the new planet, r' its radius and d' its density. The acceleration due to gravity on the surface of the new planet is
g' =  \frac{GM'}{r'^2} (1)
so we need to find M' and r'.

The problem says the radius of the new planet is twice the Earth's radius: 
r'=2r (2)
and that its density is 2/3 of Earth's density:
d'= \frac{2}{3} d
so the mass M' of the new planet is, with respect to the Earth's mass:
M' = d'V' = \frac{4}{3} \pi d' (r')^3 =  \frac{4}{3} \pi ( \frac{2}{3}d) (2r)^3 = ( \frac{4}{3} \pi d r^3 )( \frac{16}{3}) =  \frac{16}{3} M (3)

And if we substitute (2) and (3) into (1), we find the gravitational acceleration on the surface of the new planet:
g'= \frac{G( \frac{16}{3}M) }{(2r)^2}=  \frac{GM}{r^2}  \frac{4}{3} =  \frac{4}{3}g
And since g=9.81 m/s^2, we find
g'=  \frac{4}{3}(9.81 m/s^2)=13.1 m/s^2
8 0
3 years ago
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